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2010 ◽  
Vol 259 ◽  
pp. 012025 ◽  
Author(s):  
S A Bonometto ◽  
L Casarini ◽  
A V Macciò ◽  
G Stinson

2006 ◽  
Vol 88 (4) ◽  
pp. 043109 ◽  
Author(s):  
M. H. M. van Weert ◽  
O. Wunnicke ◽  
A. L. Roest ◽  
T. J. Eijkemans ◽  
A. Yu Silov ◽  
...  

2002 ◽  
Vol 579 (1) ◽  
pp. 76-82 ◽  
Author(s):  
Stephen D. Landy ◽  
Alexander S. Szalay

2002 ◽  
Vol 80 (1) ◽  
pp. 40-42 ◽  
Author(s):  
Daxing Han ◽  
Guozhen Yue ◽  
Keda Wang ◽  
Jonathan Baugh ◽  
Yue Wu ◽  
...  

1999 ◽  
Vol 117 (1) ◽  
pp. 40-55 ◽  
Author(s):  
D. P. Schneider ◽  
Maarten Schmidt ◽  
J. E. Gunn
Keyword(s):  

1996 ◽  
Vol 168 ◽  
pp. 109-116 ◽  
Author(s):  
C.J. Cesarsky ◽  
D. Elbaz

Detailed observations in the optical do not allow to discriminate between the following scenarii of galaxy formation:- synchronous formation at large redshift (z > 7).- hierarchical merging, down to z ≤ 1, of proto-galactic lumps formed at very high redshift (≈ 10).- galaxy formation at low z (≈ 2-5), but partially obscured by dust.More than 1500 galaxies in a field of 2.6′ × 4.6′ were detected by Tyson (1988) with CCD images in the B band. These deep counts of galaxies revealed the presence of an unexpectedly large population of blue galaxies, corresponding to a number excess of 3 to 5 times more galaxies at B > 23 than one can expect from the local luminosity function. These objects lie apparently at moderate redshift (z = 0.3 for B = 23–24) as shown by spectroscopy of B-selected galaxies (Collesset al.1990).


1995 ◽  
Vol 34 (S1) ◽  
pp. 191 ◽  
Author(s):  
Akira Yamashita ◽  
Tohru Maruno ◽  
Takayoshi Hayashi

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